... ma s s ejections and collisions of mass shells which produce bright radiating shocks. 15y12-Prosper p. 69 SN IIn structure, Chugai, SB ea'04 (photosphere) 15y12-Prosper p. 70 Shocks in SNe IIn A long living shock: an example for SN1994w of type IIn ...
... solar atmosphere at all levels from the photosphere up to the uppermost regions of ... and for electromagnetic fields on the photosphere always were and remain to be ... data about magnetic fields on the photosphere, data about sunspots and filaments ...
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Ссылки http://www.iki.rssi.ru/people/vcr2004.pdf -- 919.5 Кб -- 23.12.2004
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Ссылки http://www.kosmofizika.ru/buri/vesel2.pdf -- 919.5 Кб -- 31.10.2005
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Ссылки http://solarwind.cosmos.ru/vcr.pdf -- 919.5 Кб -- 02.11.2004 Похожие документы
... For example, in the case of the extremely active CTTS RU Lup, the accretion luminosity is almost 10 times larger than the bolometric luminosity of the underlying photosphere. ...
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Ссылки http://www.sai.msu.ru/dept/adm/lamzin/aah2516.pdf -- 202.4 Кб -- 28.09.2012
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Ссылки http://sai.msu.ru/dept/adm/lamzin/aah2516.pdf -- 202.4 Кб -- 28.09.2012 Похожие документы
... This takes in the measurement of physical parameters of the solar atmosphere, such as magnetic fields, density, temperature, and energy distribution of electrons and ions in the photosphere, chromosphere and corona. ...
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Ссылки http://www.princetonastronomy.org/newsletters/02_2004sidereal.pdf -- 536.0 Кб -- 02.02.2004 Похожие документы
... This is necessary, for instance, in the study of the generalized Ohm's law which is applied in the investigation of physical processes in weakly-ionized plasmas, e.g., in the solar photosphere and prominences. ...